Geologic Map of Three Sisters Volcanic Cluster, Cascade Range, Oregon by Wes Hildreth, Judy Fierstein, and Andrew T
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Geoscience and a Lunar Base
" t N_iSA Conference Pubhcatmn 3070 " i J Geoscience and a Lunar Base A Comprehensive Plan for Lunar Explora, tion unclas HI/VI 02907_4 at ,unar | !' / | .... ._-.;} / [ | -- --_,,,_-_ |,, |, • • |,_nrrr|l , .l -- - -- - ....... = F _: .......... s_ dd]T_- ! JL --_ - - _ '- "_r: °-__.......... / _r NASA Conference Publication 3070 Geoscience and a Lunar Base A Comprehensive Plan for Lunar Exploration Edited by G. Jeffrey Taylor Institute of Meteoritics University of New Mexico Albuquerque, New Mexico Paul D. Spudis U.S. Geological Survey Branch of Astrogeology Flagstaff, Arizona Proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and held at the Lunar and Planetary Institute Houston, Texas August 25-26, 1988 IW_A National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1990 PREFACE This report was produced at the request of Dr. Michael B. Duke, Director of the Solar System Exploration Division of the NASA Johnson Space Center. At a meeting of the Lunar and Planetary Sample Team (LAPST), Dr. Duke (at the time also Science Director of the Office of Exploration, NASA Headquarters) suggested that future lunar geoscience activities had not been planned systematically and that geoscience goals for the lunar base program were not articulated well. LAPST is a panel that advises NASA on lunar sample allocations and also serves as an advocate for lunar science within the planetary science community. LAPST took it upon itself to organize some formal geoscience planning for a lunar base by creating a document that outlines the types of missions and activities that are needed to understand the Moon and its geologic history. -
Qiao Et Al., Sosigenes Pit Crater Age 1/51
Qiao et al., Sosigenes pit crater age 1 2 The role of substrate characteristics in producing anomalously young crater 3 retention ages in volcanic deposits on the Moon: Morphology, topography, 4 sub-resolution roughness and mode of emplacement of the Sosigenes Lunar 5 Irregular Mare Patch (IMP) 6 7 Le QIAO1,2,*, James W. HEAD2, Long XIAO1, Lionel WILSON3, and Josef D. 8 DUFEK4 9 1Planetary Science Institute, School of Earth Sciences, China University of 10 Geosciences, Wuhan 430074, China. 11 2Department of Earth, Environmental and Planetary Sciences, Brown University, 12 Providence, RI 02912, USA. 13 3Lancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UK. 14 4School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, 15 Georgia 30332, USA. 16 *Corresponding author E-mail: [email protected] 17 18 19 20 Key words: Lunar/Moon, Sosigenes, irregular mare patches, mare volcanism, 21 magmatic foam, lava lake, dike emplacement 22 23 24 25 1/51 Qiao et al., Sosigenes pit crater age 26 Abstract: Lunar Irregular Mare Patches (IMPs) are comprised of dozens of small, 27 distinctive and enigmatic lunar mare features. Characterized by their irregular shapes, 28 well-preserved state of relief, apparent optical immaturity and few superposed impact 29 craters, IMPs are interpreted to have been formed or modified geologically very 30 recently (<~100 Ma; Braden et al. 2014). However, their apparent relatively recent 31 formation/modification dates and emplacement mechanisms are debated. We focus in 32 detail on one of the major IMPs, Sosigenes, located in western Mare Tranquillitatis, 33 and dated by Braden et al. -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
Deschutes National Forest
Deschutes National Forest Summer Trail Access and Conditions Update KNOW BEFORE YOU GO! Updated July 13, 2013 Summer Trail Highlights Summer weather, high summer/holiday use at many recreation sites and trails. Remaining snow limited to South Sister, Broken Top, Road 370 and a few patches on trails and the volcanoes above 6,000’ along the Crest. Reports of heavy blowdown (50+ trees/mile) on some trails. Wilderness Permits required. Broken Top TH and 370 Road from Todd Lake to Road 4601 are blocked by snow and closed until determined safe. June 29 photo from Broken Top. Nearly all Wilderness Tumalo Falls road open to vehicle trails are snow free with a few patches likely remaining traffic. North Fork Trail is cleared of along the PCT and on climber trails and routes up the blow down; open to bikers uphill only. volcano peaks. 16 Road and Three Creek Lakes are open and snow free. Tumalo Mt. Trail may yet have a patch or two of snow but very passible. Green Lks/Moraine Lks Trails are snow free with light blowdown. PCT has patchy snow above 6,000’ with some trail clearing in progress. Mosquito populations are highly variable with some backcountry lakes and riparian areas at high levels. Go prepared with your Ten Essential Systems: Navigation (map and compass) Sun protection (sunglasses/sunscreen) Ongoing Suttle Lake trail project with Deschutes NF Trail Insulation (extra clothing) Crew constructing one of many rock retaining walls. For Illumination (headlamp/flashlight) Your safety, please use caution and leash dogs when First-aid supplies approaching trail crews working the various trails on the Fire(waterproofmatches/lighter/candles) Deschutes. -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
Production and Saturation of Porosity in the Lunar Highlands from Impact Cratering
The fractured Moon: Production and saturation of porosity in the lunar highlands from impact cratering The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Soderblom, Jason M., et al. “The Fractured Moon: Production and Saturation of Porosity in the Lunar Highlands from Impact Cratering.” Geophysical Research Letters, vol. 42, no. 17, Sept. 2015, pp. 6939–44. © 2015 American Geophysical Union As Published http://dx.doi.org/10.1002/2015GL065022 Publisher American Geophysical Union (AGU) Version Final published version Citable link http://hdl.handle.net/1721.1/118615 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. PUBLICATIONS Geophysical Research Letters RESEARCH LETTER The fractured Moon: Production and saturation 10.1002/2015GL065022 of porosity in the lunar highlands Key Points: from impact cratering • The relation between impact-generated porosity and crater size is quantified Jason M. Soderblom1, Alexander J. Evans2, Brandon C. Johnson1, H. Jay Melosh3, Katarina Miljković1,4, • Impacts into highly porous targets 5 6 7 8 3 result in positive gravity anomalies Roger J. Phillips , Jeffrey C. Andrews-Hanna , Carver J. Bierson , James W. Head III , Colleen Milbury , 9 7 1 2,10 11 • The cratering record of the oldest Gregory A. Neumann , Francis Nimmo , David E. Smith , Sean C. Solomon , Michael M. Sori , lunar surfaces is preserved in the -
Cascades Volcano Observatory Monitoring Cascade Volcanoes
Cascades Volcano Observatory Monitoring Cascade Volcanoes http://volcanoes.usgs.gov/observatories/cvo/cvo_monitoring.html About CVO Monitoring Cascade Volcanoes Volcano Updates Volcano eruption forecasting relies on several disciplines of volcanology. Hazards Active volcanoes are complex natural systems, Monitoring and understanding a volcano's behaviors requires the attention of specialists from many science Seismicity disciplines. It demands a combination of current Deformation knowledge about magma systems, tectonic plate motion, volcano deformation, earthquakes, gases, Volcanic Gas chemistry, volcano histories, processes, and Lahar Detection hazards. Hydrothermal No single tool or technique can adequately monitor or predict volcanic behaviors. Therefore, Innovative Techniques volcanologists rely on an assortment of instruments and techniques to monitor volcanic unrest. This CVO Education requires placement of monitoring instruments both Prepare close to and far away from the primary source of eruptive activity (e.g. in a crater, on the crater rim, Multimedia and on the volcano's flanks). By placing sensitive monitoring instruments at hazardous volcanoes in Regional Volcanism Helicopter dropping off monitoring equipment at Mount St. advance of the unrest, the USGS CVO helps to Helens, Washington. ensure that communities at risk can be forewarned with sufficient time to prepare and implement response plans and mitigation measures. Recommendations for the numbers and types of ground-based sensors were made by an interdisciplinary team of scientists as part of planning for the National Volcano Early Warning System. CVO uses these recommendations to plan monitoring improvements throughout the Cascades. You can watch interviews with volcano scientists (Web Shorts) about their research and monitoring efforts and videos about volcano monitoring techniques in the Multimedia section of this website. -
POLYGONAL IMPACT CRATERS on CHARON. C.B. Beddingfield1,2, R
51st Lunar and Planetary Science Conference (2020) 1241.pdf POLYGONAL IMPACT CRATERS ON CHARON. C.B. Beddingfield1,2, R. Beyer1,2, R.J. Cartwright1,2, K. Singer3, S. Robbins3, S.A. Stern3, V. Bray4, J.M. Moore2, K. Ennico2, C.B. Olkin3, J.R. Spencer3, H.A. Weaver5, L.A. Young3, A.Verbiscer6, J. Parker3, and the New Horizons Geology, Geophysics, and Imaging (GGI) Team; 1SETI In- stitute, Mountain View, CA, 2NASA Ames Research Center, Mountain View, CA ([email protected]), 3Southwest Research Institute, Boulder, CO, 4University of Arizona, Tucson, AZ, 5John Hopkins University Applied Physics Laboratory, Laurel, MD, 6University of Virginia, Charlottesville, VA. Introduction: Polygonal impact craters (PICs) re- flect pre-existing extensional and strike-slip faults and fractures in the target material [e.g. 1-9]. PIC straight rim segments therefore can provide important infor- mation for deciphering the tectonic histories of plane- tary bodies [e.g. 8]. The only known PIC formation mechanism is the presence of pre-existing sub-vertical structures within the target material [e.g. 5, 7, 11-13]. In contrast, circular impact craters (CICs) are in- ferred to result from impact events in non-tectonized target material. CICs can also form in pre-fractured tar- get material if the fractures are widely or closely spaced, if the fracture system is highly complex, or if the target material is covered by a thick layer of non-cohesive sed- iment that limits interactions between the impactor and the underlying bedrock/ice [e.g. 14]. Consequently, PICs and CICs are useful tools to distinguish between Fig. -
Volcanic Vistas Discover National Forests in Central Oregon Summer 2009 Celebrating the Re-Opening of Lava Lands Visitor Center Inside
Volcanic Vistas Discover National Forests in Central Oregon Summer 2009 Celebrating the re-opening of Lava Lands Visitor Center Inside.... Be Safe! 2 LAWRENCE A. CHITWOOD Go To Special Places 3 EXHIBIT HALL Lava Lands Visitor Center 4-5 DEDICATED MAY 30, 2009 Experience Today 6 For a Better Tomorrow 7 The Exhibit Hall at Lava Lands Visitor Center is dedicated in memory of Explore Newberry Volcano 8-9 Larry Chitwood with deep gratitude for his significant contributions enlightening many students of the landscape now and in the future. Forest Restoration 10 Discover the Natural World 11-13 Lawrence A. Chitwood Discovery in the Kids Corner 14 (August 4, 1942 - January 4, 2008) Take the Road Less Traveled 15 Larry was a geologist for the Deschutes National Forest from 1972 until his Get High on Nature 16 retirement in June 2007. Larry was deeply involved in the creation of Newberry National Volcanic Monument and with the exhibits dedicated in 2009 at Lava Lands What's Your Interest? Visitor Center. He was well known throughout the The Deschutes and Ochoco National Forests are a recre- geologic and scientific communities for his enthusiastic support for those wishing ation haven. There are 2.5 million acres of forest including to learn more about Central Oregon. seven wilderness areas comprising 200,000 acres, six rivers, Larry was a gifted storyteller and an ever- 157 lakes and reservoirs, approximately 1,600 miles of trails, flowing source of knowledge. Lava Lands Visitor Center and the unique landscape of Newberry National Volcanic Monument. Explore snow- capped mountains or splash through whitewater rapids; there is something for everyone. -
Information Circular 41: Origin of Cascade Landscapes
111ackin I CdrlJ .rc-1J ORIGIN OF CASCADE LANDSCAPES ---=-~--=---------=---- FRONTISPIECE Picket Range in upper Skagit area, Northern Cascade Mountains. Snowfields occupy a former ice-filled cirque. Grass is enroaching on ice-polished rock surfaces. State of Washington DANIEL J. EVANS, Governor Department of Conservation ROY MUNDY, Director DIVISION OF MINES AND GEOLOGY MARSHALL T. HUNTTING, SupervisoT Information Circular No. 41 ORIGIN OF CASCADE LANDSCAPES By J. HOOVER MACKIN and ALLENS. CARY STATE PRINTING PLANT, OLYMPIA, WASHINGTON 1965 For sale by Department of Conservation, Olympia, Washington. Price, 50 cents. FOREWORD The Cascade Range has had an important influence on the lives of a great many people ever since man has inhabited the Northwest. The mountains were a barrier to Indian travel; they were a challenge to the westward migration of the early settlers in the area; they posed serious problems for the early railroad builders; and they still constitute an obstruction to east-west travel. A large part of the timber, mineral, and surface water resources of the State come from the Cascades. About 80 percent of the area covered by glaciers in the United States, exclusive of Alaska, is in the Cascades of Washington. This region includes some of the finest mountain scenery in the country and is a popular outdoor recreation area. The Cascade Range is a source of economic value to many, a source of pleasure to many others, and a problem or source of irritation to some. Regardless of their reactions, many people have wondered about the origin of the mountains How and when did the Cascades come into being, and what forces were responsible for the construction job? -This report, "Origin of Cascade Landscapes," gives the answers to these questions. -
Chapter 15 Comparative Phylogeography of North- Western North America: a Synthesis
Chapter 15 Comparative phylogeography of north- western North America: a synthesis S. J. Brunsfeld,* J. Sullivan,†D. E. Soltis‡and P. S. Soltis§ Introduction Phylogeography is concerned with the principles and processes that determine the geographic distributions of genealogical lineages, within and among closely related species (Avise et al. 1987;Avise 2000).Although this field of study is very new (only a little more than a decade has passed since the term ‘phylogeography’was first coined; see Avise et al. 1987),the scientific literature in this research area is now voluminous. To date, most phylogeographic investigations of natural populations have focused on muticellular animals (Hewitt 1993; Patton et al. 1994; daSilva & Patton 1998; Eizirik et al. 1998;Avise 2000; Hewitt 2000; Schaal & Olsen 2000; Sullivan et al. 2000). This bias is due in large part to the ready availability of population-level genetic markers afforded by the animal mitochondrial genome. The more slowly evolving chloroplast genome,in contrast,often does not provide sufficient variation to reconstruct phylogeny at the populational level (Soltis et al. 1997; Schaal et al. 1998; Schaal & Olsen 2000). Phylogeographic data have accumulated so rapidly for animal taxa that it has been possible to compare phylogeographic structure among codistributed species. In fact, one of the most profound recent contributions of molecular phylogeography is the construction of regional phylogeographic perspec- tives that permit comparisons of phylogeographic structure among codistributed species, and subsequent integration of genealogical data with independent biogeo- graphic and systematic data. Probably the best-known regional phylogeographic analysis for North America involves animals from the southeastern USA (reviewed in Avise 2000). -
Diamond Craters Oregon's Geologic
Text by Ellen M. Benedict, 1985 Features at stops correspond to points on a clock ago, a huge mass of hot gases, volcanic ashes, bits face. Imagine that you are standing in the middle of a of pumice and other pyroclastics (fire-broken rock) Travel And Hiking Hints clock face. Twelve o’clock is the road in front of you violently erupted. The blast – greater than the May and 6 o’clock the road behind. If you always align the 18, 1980, eruption of Mt. St. Helens – deposited a Diamond Craters is located in the high desert country clock face with the road, you should be able to locate layer of pyroclastics 30 to 130 feet thick over an area about 55 miles southeast of Burns, Oregon. It’s an the features. almost 7,000 square miles! isolated place and some precautions should be taken . when traveling in the area. Start Tour. Mileage begins halfway Pyroclastics are between milepost 40 and 41 on State normal behavior Diamond Craters has no tourist facilities. The nearest Highway 205 at the junction to Diamond. for magmas place where gasoline is sold is at Frenchglen. Turn left. (subsurface That’s the opinion held by scores of molten rocks) Keep your scientists and educators who have visited Diamond, Oregon, a small ranching community, was of rhyolitic (a vehicle on named in 1874 for Mace McCoy’s Diamond brand. volcanic material and studied the area. It has the “best and hard-packed The nearby craters soon became known as Diamond related to granite) most diverse basaltic volcanic features in the road surfaces Craters.